Go with the flow: The self-similar and non-linear behaviour of large-scale in- and outflows and the impact of accretion shocks from galaxies to galaxy clusters

Open Access

Fig. 15.

Metallicity of the net (mean) inflow and outflow as a function of mass at five radii for the full halo sample. As in Fig. 14, the spread within each mass bin is indicated by the vertical distributions. As in Fig. 14 the cut-off in the high-mass–large radius range does not indicate zero metallicity.

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